Polarizing Microscope IMP-2100 Series equipped with a high degree of sensitivity and best suited for anisotropic (mineral) specimens such as geology, minerals, metallurgy, university teaching laboratories, and other sectors. Built-in bertrand lens, polarizer, and analyzer, 360° rotatable round stage, filter, condenser, etc. The trinocular viewing head with extra wild field eyepieces and has excellent strain-free plan achromatic: 5X/0.12/∞/-15.5 mm, 10X/0.25/∞/-10.0 mm, 20X/0.4/∞/0-5.8 mm, 50X/0.75/∞/0-0.32 mm, 100X/0.8/∞/0-2 mm objectives, and each eye tube has interpupillary adjustment. This series is capable of provid
Description
Specification
Technical
Polarizing Microscope IMP-2100 Series equipped with a high degree of sensitivity and best suited for anisotropic (mineral) specimens such as geology, minerals, metallurgy, university teaching laboratories, and other sectors. Built-in bertrand lens, polarizer, and analyzer, 360° rotatable round stage, filter, condenser, etc. The trinocular viewing head with extra wild field eyepieces and has excellent strain-free plan achromatic: 5X/0.12/∞/-15.5 mm, 10X/0.25/∞/-10.0 mm, 20X/0.4/∞/0-5.8 mm, 50X/0.75/∞/0-0.32 mm, 100X/0.8/∞/0-2 mm objectives, and each eye tube has interpupillary adjustment. This series is capable of providing strong images with a broad field of view, the multipurpose and perfect for basic studies of samples properties. Come with 24V/100W Halogen lamp reflected lights, allowing samples to be illuminated for a more comprehensive field of view. Accomplished with the help of particular devices known as retardation plates and optical compensators. The first-order retardation plate is used in optical path differences ranging from a fraction of a wavelength up to several wavelengths. This flexible and multipurpose tool is known by different names, comprising a red plate, red-one plate, lambda (λ) plate, gypsum plate, selenite plate, sensitive violet, or simply a color tint plate and quartz wedge plate is a simple, semi-quantitative optical compensator used to examine optical path differences in a wide range of samples by the quartz wedge. Built-in a crystalline block of quartz provide a parallel or perpendicular optical axis to the edge of the birefringent crystal.
Accomplished with the help of particular devices known as retardation plates and optical compensators.
Infinite strain free plan achromatic objective, and Backward quintuple nosepiece
Gypsum λ Slip, First Class Red, 1/4λ Slip, (â… -â…£ Class) Quartz Wedge optical compensate system
High point wild field EW10×/22mm and Plan eyepiece with scale of crosshair, gridding eyepieces
Coaxial coarse & fine adjustment, range 32mm, fine division 0.001mm, coarse stroke 37.7mm per rotation, fine stroke 0.1mm per rotation
Polarizing rotatable stage of length 170mm, center adjustable, 360° scale, minimum division 1°, minimum reading vernier scale 6 to 45° stop knob
N.A.0.9/0.13 swing out condenser
24V/100W Halogen lamp reflected light source
Trinocular 30° inclined and a 360° rotatable head with interpupillary distance 48 to 75 mm and
Small foot print and light weight
Easy operating with ergonomic design
Excellent image quality with an infinite optical system
Optional accessories video adaptor and filters
Built-in a crystalline block of quartz provide parallel or perpendicular optical axis to the edge of the birefringent crystal
Technical Specifications
Model
IMP-2101
Type
Advanced Polarizing Microscope
Viewing Head
Trinocular head, Inclined at 30°, Interpupillary 48-75mm
Optical System
Infinite
Focusing
Coaxial coarse & fine adjustment, range 32mm, fine division 0.001mm, coarse stroke 37.7mm per rotation, fine stroke 0.1mm per rotation
Eyepiece
Plan eyepiece EW10X22mm and Plan eyepiece with scale of crosshair, Plan eyepiece with crosshair, Plan eyepiece with gridding
Nosepiece
Backward quintuple
Objective
Strain-Free Plan Achromatic :5X/0.12/∞/, 15.5mm,10X/0.25/∞/-,10.0mm,20X/0.4/∞/0, 5.8 mm, 50X/0.75/∞/0,0.32mm, 100X/0.8/∞/0,2mm